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The movement of small particulate matter in the early solar system and the formation of satellitesThe motions of the abundant small particulate matter in the early solar system are discussed. The effects of gas drag and resonance effects of perturbing forces could have led to accretion and differentiation of the matter. The composition of the moon and the existence of the rings of Saturn can be explained on the basis of the assembly of small particulate matter in satellite orbits around the planets.
Document ID
19750037525
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Gold, T.
(Cornell University Ithaca, N.Y., United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1974
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Highlights of astronomy. Volume 3
Location: Sydney
Country: Australia
Start Date: August 21, 1973
End Date: August 30, 1973
Accession Number
75A21597
Funding Number(s)
CONTRACT_GRANT: NGL-33-010-005
Distribution Limits
Public
Copyright
Other

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